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A. Kryszczynska Et Al.: Do Slivan States Exist in Other Asteroid

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A. Kryszczyn´ska et al.: Do Slivan States exist in other asteroid families? I. Table 2. Physical data of the Flora family asteroids. Objects observed within this survey are marked with boldface, A indicates data from AcuA, diameters if not given by AcuA are calculated from MPC absolute magnitude H and albedo, taxonomic types from (Neese 2010) are indicated with 1, types from SDSS-based Asteroid Taxonomy (Hasselman et al. 2011) are marked with 2, and Alvarez-Candal et al. (2006) marked with 3. Asteroid D[km] H[mag] A[mag] pv P[h] f[1/d] type HCM WAM HCM 2010 8 Flora 138.31A 6.49A 0.11 0.235A 12.865 1.8655 S, Sw 1 + + + 9 Metis 166.48A 6.28A 0.36 0.213A 5.079 4.7253 S 1 + 43 Ariadne 58.75A 7.93A 0.66 0.347A 5.762 4.1652 S, Sk, Sq 1 + + + 244 Sita 11.60A 12.20A 0.82 0.176A 129.51 0.1853 Sa, Sw 1 + 281 Lucretia 12.27A 12.02A 0.30 0.185A 4.349 5.5183 SU 1 + + 291 Alice 13.19A 11.45A 0.50 0.270A 4.316 5.5607 S 1 + + 298 Baptistina 20.53A 11.00A 0.15 0.170A 16.23 1.4787 X, Xc 1 + + + 315 Constantia 6.089 13.20 0.57 0.25 5.345 4.4902 – + + 352 Gisela 26.76A 10.01A 0.66 0.249A 7.4796 3.2087 S,Sl, S0, Sw 1 + + + 364 Isara 28.78A 9.86A 0.65 0.244A 9.1570 2.6209 S, S0 1 + + 367 Amicitia 16.78A 10.70A 0.70 0.343A 5.055 4.7478 S 3 + 376 Geometria 34.80A 9.49A 0.19 0.235A 7.734 3.1032 S 1,2 + 428 Monachia 21.79A 11.50A 0.25 0.097A 3.6342 6.6039 X 3 + + 453 Tea 24.07A 10.60A 0.12 0.176A 6.811 3.5237 S 1 + + 540 Rosamunde 19.12A 10.76A 0.60 0.265A 9.349 2.5671 S 1 + + + 553 Kundry 9.93A 12.20A 0.52 0.237A 12.381 1.9200 S 1 + + + 685 Hermia 11.46A 11.80A 0.90 0.280A 50.40 0.4768 S 1 + + + 700 Auravictrix 15.19A 11.20A 0.44 0.263A 6.075 3.9506 S 1,3 + + + 711 Marmulla 11.90A 11.90A 0.04 0.224A 2.88 8.3333 A 3 + + + 728 Leonisis 7.32 12.80 0.20 0.25 5.5783 4.3024 A,S 1,2 + + + 736 Harvard 17.92A 11.64A 0.32 0.122A 6.7 3.5821 S 1 + 770 Bali 16.07A 10.93A 0.65 0.304A 5.8199 4.1238 S 1 + 800 Kressmannia 14.23A 11.61A 0.34 0.202A 4.4610 5.3794 S 1 + + + 802 Epyaxa 8.027 12.60 0.70 0.25 4.389 5.4645 – + + 810 Atossa 8.405 12.50 0.55 0.25 4.385 5.4732 A 3 + 825 Tanina 13.06A 11.50A 0.50 0.278A 6.9398 3.4583 SR,S 1 + + 827 Wolfiana 15.04 13.20 0.19 0.041 4.0 6.0000 D 3 + + 836 Jole 5.06 13.6 0.37 0.25 9.615 2.4961 S 2 + 841 Arabella 8.027 12.60 0.25 0.25 3.352 7.1599 – + + + 851 Zeissia 12.81A 11.62A 0.38 0.248A 9.34 2.5696 S 1 + + 864 Aase 5.76A 12.87A 0.20 0.378A 3.2325 7.4246 S 1 + + 883 Matterania 8.027 12.60 0.42 0.25 5.64 4.2553 S 1 + + + 901 Brunsia 11.61A 11.35A 0.27 0.480A 3.136 7.6523 S 1 + 905 Universitas 11.84A 11.59A 0.28 0.30A 14.238 1.6856 S 1 + + + 913 Otila 11.32A 11.90A 0.10 0.245A 4.8719 4.9262 Sa, Sw 1 + + + 915 Cosette 12.31A 11.70A 0.52 0.247A 4.4701 5.3690 S 1,3 + + + 929 Algunde 10.70A 12.10A 0.14 0.242A 3.310 7.2503 S, Sl 1 + + + 935 Clivia 7.18A 12.90A 0.13 0.247A 3.6222 6.6258 – + + 937 Bethgea 12.69A 11.83A 0.20 0.203A 7.539 3.1834 S 1 + + 951 Gaspra 15.68A 11.46A 1.00 0.189A 7.0420 3.4081 S 1 + + + 956 Elisa 8.00 12.1 0.36 0.4 16.50 1.4545 V 1 + 960 Birgit 6.991 12.90 0.27 0.25 8.85 2.7119 A 3 + 963 Iduberga 10.38A 12.49A 0.34 0.165A 3.0341 7.9101 S 1 + + 967 Helionape 13.55A 12.10A 0.13 0.142A 3.232 7.4257 – + + + 1016 Anitra 11.08 11.90 0.28 0.25 5.9288 4.0480 S 1 + + + 1055 Tynka 8.95A 12.00A 0.09 0.35A 11.893 2.0180 S 1 + + 1056 Azalea 13.07A 11.70A 0.72 0.223A 15.03 1.5968 S 1 + + + 1060 Magnolia 7.665 12.70 0.25 0.25 2.9108 8.2452 S 1,2 + + + 1088 Mitaka 13.35A 11.39A 0.62 0.276A 3.0353 7.9070 S 1 + + 1117 Reginita 12.149 11.70 0.30 0.25 2.9464 8.1455 S 1,2 + 1120 Cannonia 9.920A 12.80A 0.16 0.137A 3.8160 6.2893 – + 1130 Skuld 10.24A 12.10A 0.53 0.244A 4.8079 4.9918 S,Sl 1 + + 1133 Lugduna 10.47A 12.22A 0.45 0.208A 5.478 4.3812 S 1 + + 1185 Nikko 12.56A 12.09A 0.50 0.164A 3.79 6.3324 S 1 + + + 1188 Gothlandia 12.11A 11.70A 0.70 0.252A 3.4917 6.8734 S 1 + + + 1219 Britta 11.76A 11.94A 0.73 0.223A 5.5750 4.3049 S 1 + + 1225 Ariane 9.10A 12.10A 0.36 0.308A 5.5068 4.3582 – + + 1249 Rutherfordia 15.77A 11.54A 0.65 0.1720A 18.220 1.3172 S 1 + + + 1270 Datura 7.83A 12.50A 0.61 0.291A 3.359 7.1450 S 3 + + + 1314 Paula 6.7A 12.68A 0.83 0.377A 5.9498 4.0337 S 1 + + + 13 A. Kryszczyn´ska et al.: Do Slivan States exist in other asteroid families? I. Table 2. Continiued Asteroid D[km] H[mag] A[mag] pv P[h] f[1/d] type HCM WAM HCM 2010 1324 Knysna 7.32 12.80 0.08 0.25 2.5538 9.3978 Sq 1 + + 1344 Caubeta 7.32 12.80 0.21 0.25 3.1220 7.6874 S 2 + + 1376 Michelle 8.405 12.50 0.20 0.25 5.9769 4.0155 – + + 1396 Outenniqua 11.00A 12.00A 0.42 0.237A 3.0810 7.7897 S, Sl 1 + 1449 Virtanen 10.581 12.00 0.69 0.25 30.495 0.7870 S, Sl 1 + + + 1472 Muonio 9.216 12.30 0.48 0.25 8.7060 2.7567 – + + 1496 Turku 8.801 12.40 0.51 0.25 6.47 3.7094 – + + 1514 Ricouxa 8.027 12.60 0.62 0.25 10.438 2.2993 – + + 1518 Rovaniemi 8.801 12.40 0.25 0.25 5.2490 4.572 S 1 + + + 1523 Pieksamaki 19.30 12.30 0.46 0.057 5.3202 4.5111 C 3 + + + 1527 Malmquista 9.65 12.20 0.54 0.25 14.077 1.7049 S 2 + + 1562 Gondolatsch 11.12A 11.80A 0.42 0.283A 8.74 2.7460 S 1 + + + 1590 Tsiolkovskaja 12.81A 11.70A 0.30 0.232A 6.7299 3.5662 – + + + 1601 Patry 10.93A 12.32A 0.72 0.178A 5.92 4.0541 Sl 1 + + + 1602 Indiana 8.410A 12.49A 0.17 0.259A 2.6010 9.2272 S 1 + + 1619 Ueta 10.105 12.10 0.35 0.25 2.7180 8.8300 S 1,2 + + 1622 Chacornac 10.27A 12.2A 0.25 0.224A 12.206 1.9662 S 1 + + + 1631 Kopff 9.580A 12.20A 0.41 0.259A 6.6830 3.5912 – + + 1666 Van Gent 8.405 12.50 0.30 0.25 4.1660 5.7609 – + + 1667 Pels 10.62A 12.10A 0.25 0.232A 3.2681 7.3437 Sa,Sw 1 + 1675 Simonida 12.16A 11.90A 0.58 0.211A 5.2885 4.5381 – + + + 1682 Karel 4.80A 12.90A 0.47 0.531A 3.3750 7.1111 – + + + 1738 Oosterhoff 7.62A 12.30A 0.54 0.370A 4.4470 5.3969 S 1 + + 1785 Wurm 6.089 13.20 0.29 0.25 3.2693 7.3410 S 1 + + + 1790 Volkov 8.670A 12.50A 0.09 0.241A 10.742 2.2342 – + + + 1793 Zoya 8.027 12.60 0.72 0.25 5.74 4.1812 S, SL 1 + 1806 Derice 10.14A 12.00A 0.19 0.282A 3.2240 7.4442 S, SL 1 + + + 1807 Slovakia 8.801 12.40 1.00 0.25 308.0 0.0779 S, Sqw 1 + 1829 Dawson 9.67A 12.50A 0.28 0.189A 4.254 5.6417 S 2 + + 1855 Korolev 8.405 12.50 0.75 0.25 4.6500 5.1613 – + + + 2017 Wesson 8.027 12.60 0.61 0.25 3.4158 7.0262 S,X 1,3 + + + 2036 Sheragul 7.0A 12.70A 0.71 0.30A 5.45 4.4037 A 2 + 2080 Jihlava 7.32 12.80 0.15 0.25 2.7088 8.8600 – + 2093 Genichesk 12.29 13.28 0.24 0.057 11.028 2.1763 C 1 + + + 2094 Magnitka 9.910A 12.00A 0.86 0.285A 6.1100 3.9280 – + + + 2156 Kate 8.801 12.40 0.91 0.25 5.6230 4.2682 A 1,2 + 2283 Bunke 16.05 12.70 0.07 0.057 4.3 5.5814 C 2 + 2445 Blazhko 10.581 12.00 0.57 0.25 3.6200 6.6298 S 2 + + + 2460 Mitlincoln 9.216 12.30 0.20 0.25 2.8277 8.4875 L 2 + 2510 Shandong 7.09A 12.60A 0.44 0.345A 3.4963 6.8644 S 1 + + 2647 Sova 8.405 12.50 0.35 0.25 9.3660 2.5625 – + + + 2709 Sagan 6.676 13.00 0.36 0.25 5.2580 4.5645 S 1 + 2768 Gorky 10.105 12.10 0.51 0.25 4.5070 5.3250 A 3 + + + 2839 Annette 7.665 12.70 0.92 0.25 10.457 2.2951 – + 2841 Puijo 7.665 12.70 0.03 0.25 3.5450 6.7701 S, Sk 1 + + + 2853 Harvill 7.32 12.8 0.65 0.25 6.30 3.8095 – + 2961 Katsurahama 6.676 13.0 0.28 0.25 2.937 8.1716 S 1 + + + 3105 Stumpff 7.430A 13.10A 0.35 0.185A 5.0369 4.7648 S, Sl 1 + + 3144 Brosche 4.619 13.80 0.60 0.25 3.30 7.2727 – + + 3165 Mikawa 8.027 12.60 0.25 0.25 5.100 4.7244 S 2 + + + 3410 Vereshchagin 5.303 13.50 0.10 0.25 2.5780 9.3095 S 2 + + + 3411 Debetencourt 5.815 13.30 0.43 0.25 9.9300 2.4169 – + + 3455 Kristensen 7.665 12.70 0.38 0.25 8.1110 2.9589 – + 3533 Toyota 9.90 12.70 0.18 0.15 2.9810 8.0510 Xk, X 1,2 + + + 3573 Holmberg 7.320 12.80 1.03 0.25 6.5431 3.6680 S, Sr 1,2 + + 3722 Urata 8.027 12.60 0.58 0.25 5.5670 4.3111 – + + 3763 Qianxuesen 8.260A 12.50A 0.31 0.259A 3.8840 6.1792 L 2 + + 3825 Nurnberg 7.665 12.70 0.71 0.25 4.0300 5.9553 – + + + 3850 Peltier 4.19 13.50 0.10 0.40 2.4289 9.8810 V 1 + 3953 Perth 5.064 13.60 0.92 0.25 5.083 4.7216 – + 3956 Caspar 7.32 12.80 0.13 0.25 2.7707 8.6621 – + + 3986 Rozhkovskij 7.665 12.70 0.35 0.25 3.5493 6.7619 – + + 4080 Galinskij 5.815 13.30 1.01 0.25 7.3500 3.2653 – + + + 4150 Starr 7.665 12.70 0.21 0.25 4.5179 5.3122 S 2,3 + 14.
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    Astronomy & Astrophysics manuscript no. aa˙2009 c ESO 2018 August 22, 2018 A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method 1 1 1 2 3 4 5 6 7 J. Hanuˇs ∗, J. Durechˇ , M. Broˇz , B. D. Warner , F. Pilcher , R. Stephens , J. Oey , L. Bernasconi , S. Casulli , R. Behrend8, D. Polishook9, T. Henych10, M. Lehk´y11, F. Yoshida12, and T. Ito12 1 Astronomical Institute, Faculty of Mathematics and Physics, Charles University in Prague, V Holeˇsoviˇck´ach 2, 18000 Prague, Czech Republic ∗e-mail: [email protected] 2 Palmer Divide Observatory, 17995 Bakers Farm Rd., Colorado Springs, CO 80908, USA 3 4438 Organ Mesa Loop, Las Cruces, NM 88011, USA 4 Goat Mountain Astronomical Research Station, 11355 Mount Johnson Court, Rancho Cucamonga, CA 91737, USA 5 Kingsgrove, NSW, Australia 6 Observatoire des Engarouines, 84570 Mallemort-du-Comtat, France 7 Via M. Rosa, 1, 00012 Colleverde di Guidonia, Rome, Italy 8 Geneva Observatory, CH-1290 Sauverny, Switzerland 9 Benoziyo Center for Astrophysics, The Weizmann Institute of Science, Rehovot 76100, Israel 10 Astronomical Institute, Academy of Sciences of the Czech Republic, Friova 1, CZ-25165 Ondejov, Czech Republic 11 Severni 765, CZ-50003 Hradec Kralove, Czech republic 12 National Astronomical Observatory, Osawa 2-21-1, Mitaka, Tokyo 181-8588, Japan Received 17-02-2011 / Accepted 13-04-2011 ABSTRACT Context. In the past decade, more than one hundred asteroid models were derived using the lightcurve inversion method. Measured by the number of derived models, lightcurve inversion has become the leading method for asteroid shape determination.
  • Do Slivan States Exist in the Flora Family? A

    Do Slivan States Exist in the Flora Family? A

    Do Slivan states exist in the Flora family? A. Kryszczyńska, F. Colas, M. Polińska, R. Hirsch, V. Ivanova, G. Apostolovska, B. Bilkina, F. Velichko, T. Kwiatkowski, P. Kankiewicz, et al. To cite this version: A. Kryszczyńska, F. Colas, M. Polińska, R. Hirsch, V. Ivanova, et al.. Do Slivan states exist in the Flora family?. Astronomy and Astrophysics - A&A, EDP Sciences, 2012, 546, pp.A72. 10.1051/0004- 6361/201219199. hal-03123875 HAL Id: hal-03123875 https://hal.archives-ouvertes.fr/hal-03123875 Submitted on 28 Jan 2021 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. A&A 546, A72 (2012) Astronomy DOI: 10.1051/0004-6361/201219199 & c ESO 2012 Astrophysics Do Slivan states exist in the Flora family? I. Photometric survey of the Flora region A. Kryszczynska´ 1,F.Colas2,M.Polinska´ 1,R.Hirsch1, V. Ivanova3, G. Apostolovska4, B. Bilkina3, F. P. Velichko5, T. Kwiatkowski1,P.Kankiewicz6,F.Vachier2, V. Umlenski3, T. Michałowski1, A. Marciniak1,A.Maury7, K. Kaminski´ 1, M. Fagas1, W. Dimitrov1, W. Borczyk1, K. Sobkowiak1, J. Lecacheux8,R.Behrend9, A. Klotz10,11, L. Bernasconi12,R.Crippa13, F. Manzini13, R.
  • Binary Asteroid Lightcurves

    Binary Asteroid Lightcurves

    BINARY ASTEROID LIGHTCURVES Asteroid Type Per1 Amp1 Per2 Amp2 Perorb Ds/Dp a/Dp Reference 22 Kalliope B 4.1483 0.53 B a Descamps, 08 B a 86.2896 Marchis, 08 B a 4.148 86.16 Marchis, 11w 41∗ Daphne B 5.988 0.45 B s 26.4 Conrad, 08 B s 38. Conrad, 08 B s 5.987981 27.289 2.46 Carry, 18 45 Eugenia M 5.699 0.30 B a 113. Merline, 99 B a Marchis, 06 M a Marchis, 07 M a Marchis, 08 B a 5.6991 114.38 Marchis, 11w 87 Sylvia M 5.184 0.50 M a 5.184 87.5904 Marchis, 05 M a 5.1836 87.59 Marchis, 11w 90∗ Antiope B 16.509 0.88 B f 16. Merline, 00 B f 16.509 0.73 16.509 0.73 16.509 Descamps, 05 B f 16.5045 0.86 16.5045 0.86 16.5045 Behrend, 07w B f 16.505046 16.505046 Bartczak, 14 93 Minerva M 5.982 0.20 M a 5.982 0.20 57.79 Marchis, 11 107∗ Camilla M 4.844 0.53 B a Marchis, 08 B a 4.8439 89.04 Marchis, 11w M a 1.550 Marsset, 16 M s 89.096 4.91 Pajuelo, 18 113 Amalthea B? 9.950 0.22 ? u Maley, 17 121 Hermione B 5.55128 0.62 B a Merline, 02 B a Marchis, 04 B a Marchis, 05 B a 5.55 61.97 Marchis, 11w 130 Elektra M 5.225 0.58 B a 5.22 126.2 Marchis, 08 M a Yang, 14 216 Kleopatra M 5.385 1.22 M a 5.38 Marchis, 08 243 Ida B 4.634 0.86 B a Belton, 94 279 Thule B? 23.896 0.10 B s 7.44 0.08 72.2 Sato, 15 283 Emma B 6.896 0.53 B a Merline, 03 B a 6.89 80.48 Marchis, 08 324 Bamberga B? 29.43 0.12 B s 29.458 0.06 71.0 Sato, 15 379 Huenna B 14.141 0.12 B a Margot, 03 B a 4.022 2102.